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UV completeness restricts fifth-force parameters to a narrow region in scalar-tensor gravity

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2026-06-30 22:41 UTC pith:VMAFWSE2

load-bearing objection UV completeness in this O(N) scalar-tensor model carves the allowed fifth-force parameters down to a narrow wedge in the (α, λ) plane.

arxiv 2605.10338 v2 pith:VMAFWSE2 submitted 2026-05-11 gr-qc hep-phhep-th

Fifth-Force Constraints from UV-Complete Scalar-Tensor Gravity

Alfio M. Bonanno , Emiliano M. Glaviano This is my paper
classification gr-qc hep-phhep-th
keywords scalar-tensor gravityfifth forcerenormalization groupUV completenessYukawa correctionO(N) scalar multipletasymptotic safety
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved

The pith

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The paper examines an O(N) scalar multiplet nonminimally coupled to gravity and tracks its renormalization-group flow near an interacting UV-complete scaling regime. In the broken phase the radial mode produces a Yukawa correction to Newtonian gravity parametrized by strength α and range λ. Only trajectories that remain regular and reach the UV regime are permitted; these occupy a finite wedge whose image in the (α, λ) plane is a narrow allowed band. The complement of this band is therefore excluded by UV completeness alone. Because part of the excluded domain lies below present experimental bounds, future fifth-force searches can test the models directly.

Core claim

In the broken phase of an O(N) scalar multiplet nonminimally coupled to gravity, the radial mode mediates a universal Yukawa correction to Newtonian gravity with strength α and range λ. Requiring that renormalization-group trajectories remain regular and reach the interacting UV-complete scaling regime restricts the infrared data to a finite wedge. This wedge maps to a narrow region in the (α, λ) plane, so its complement is ruled out by UV completeness alone.

What carries the argument

Regular renormalization-group trajectories that connect the broken phase of the O(N) scalar-tensor theory to its interacting nonperturbative UV-complete scaling regime.

Load-bearing premise

The theory admits an interacting nonperturbative UV-complete scaling regime whose renormalization-group trajectories can be continued from the broken phase.

What would settle it

Detection of a fifth force with parameters (α, λ) lying outside the narrow UV-allowed band would show that no regular trajectory reaches the assumed UV scaling regime.

Watch this falsifier — get emailed when new claim-graph text bears on it.

If this is right

  • The allowed infrared couplings lie inside a finite wedge fixed by UV completeness.
  • This wedge projects to a narrow strip in the (α, λ) plane for the Yukawa correction.
  • Any (α, λ) values outside the strip are excluded by UV completeness without reference to experiment.
  • Future fifth-force experiments can directly probe the boundary of the UV-allowed region.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • Laboratory searches at sub-millimeter ranges corresponding to excluded λ values could falsify the UV-complete scalar-tensor scenario if a signal is found.
  • UV completeness supplies a theoretical prior that narrows the space of possible gravitational deviations independently of data.
  • Analogous RG restrictions could be derived for other scalar-tensor models once their UV fixed points are located.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit.

Referee Report

0 major / 3 minor

Summary. The manuscript analyzes the renormalization-group flow of an O(N) scalar multiplet nonminimally coupled to gravity in the vicinity of an interacting, nonperturbatively UV-complete fixed point. In the broken phase the radial mode generates a universal Yukawa correction to Newtonian gravity parametrized by strength α and range λ. The requirement that RG trajectories remain regular and reach the UV scaling regime restricts the allowed infrared data to a finite wedge in parameter space; this wedge maps to a narrow region of the (α, λ) plane whose complement is therefore excluded by UV completeness alone. Part of the excluded domain lies below present experimental bounds.

Significance. If the central mapping holds, the work supplies a purely theoretical constraint on fifth-force parameters that originates from the existence and basin of attraction of a nonperturbative UV fixed point. This constitutes a falsifiable prediction for a concrete class of scalar-tensor models and directly connects functional RG methods in gravity to laboratory-scale phenomenology. The absence of additional ad-hoc assumptions beyond the model definition and the UV-completeness requirement is a notable strength.

minor comments (3)
  1. [§3] §3 (or equivalent section containing the flow equations): the truncation ansatz and the precise definition of the radial-mode Yukawa coupling should be stated explicitly so that the mapping from the RG wedge to the (α, λ) plane can be reproduced without ambiguity.
  2. [Figure 4] Figure 4 (or the figure showing the excluded region): the experimental exclusion envelopes should be overlaid with the same line styles and color coding used in the text to facilitate direct visual comparison.
  3. [Discussion] The sentence claiming that the excluded domain 'lies below current experimental exclusion envelopes' would benefit from a quantitative statement of the fraction of the wedge that is already ruled out versus the fraction that remains testable.

Simulated Author's Rebuttal

0 responses · 0 unresolved

We thank the referee for the positive assessment of our manuscript on fifth-force constraints arising from UV-complete scalar-tensor gravity. The recommendation for minor revision is noted; we will prepare a revised version accordingly.

Circularity Check

0 steps flagged

No significant circularity; derivation self-contained

full rationale

The abstract states that UV completeness restricts IR data to a finite wedge mapping to a narrow (α,λ) region, with the complement ruled out. This follows from RG trajectories reaching an interacting UV fixed point in the broken phase, where the radial mode yields the Yukawa parameters. No quoted equation or step reduces the wedge or mapping to a fitted input, self-definition, or load-bearing self-citation by construction. The result is obtained from the flow analysis under the stated assumptions rather than presupposed, making the derivation independent of its target outputs.

Axiom & Free-Parameter Ledger

0 free parameters · 2 axioms · 0 invented entities

Ledger is inferred from the abstract only. The central claim rests on the existence of a UV fixed point and the identification of the radial mode as the mediator; no explicit free parameters or invented entities are named in the abstract.

axioms (2)
  • domain assumption Existence of an interacting nonperturbative UV-complete fixed point for the O(N) scalar multiplet nonminimally coupled to gravity
    Invoked to define the UV-completeness condition that restricts the IR wedge.
  • domain assumption The radial mode in the broken phase mediates a universal Yukawa correction to Newtonian gravity
    Used to parametrize the fifth force by α and λ.

pith-pipeline@v0.9.1-grok · 5675 in / 1446 out tokens · 39630 ms · 2026-06-30T22:41:01.067635+00:00 · methodology

0 comments
read the original abstract

We study an $O(N)$ scalar multiplet nonminimally coupled to gravity and follow its renormalization-group (RG) flow in the vicinity of an interacting, nonperturbatively UV-complete scaling regime of scalar-tensor theory. In the broken phase, the radial mode mediates a universal Yukawa correction to Newtonian gravity, parametrized by a strength $\alpha$ and range $\lambda$. Imposing UV completeness -- regular RG trajectories that reach the UV scaling regime -- restricts the infrared data to a finite wedge, which maps to a narrow region in the $(\alpha,\lambda)$ plane. Its complement is, therefore, ruled out by UV completeness alone. Remarkably, part of this theory-excluded domain lies below current experimental exclusion envelopes, so improved fifth-force searches can directly test and potentially falsify this class of UV-complete scalar-tensor models.

Figures

Figures reproduced from arXiv: 2605.10338 by Alfio M. Bonanno, Emiliano M. Glaviano.

Figure 1
Figure 1. Figure 1: FIG. 1. Renormalization-group flow in the ( [PITH_FULL_IMAGE:figures/full_fig_p003_1.png] view at source ↗
Figure 2
Figure 2. Figure 2: FIG. 2. Constraints on Yukawa-type fifth forces in the ( [PITH_FULL_IMAGE:figures/full_fig_p005_2.png] view at source ↗

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  1. Towards gauge independence in asymptotically safe quantum gravity

    hep-th 2026-07 conditional novelty 6.0

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Reference graph

Works this paper leans on

30 extracted references · 30 canonical work pages · cited by 1 Pith paper · 18 internal anchors

  1. [1]

    Phase dependence and breaking of marginality—UV- complete trajectories ariseonly afterthe flow enters the broken phase

    = 1. Phase dependence and breaking of marginality—UV- complete trajectories ariseonly afterthe flow enters the broken phase. In the symmetric phase the nongaussian couplingf 1 is exactly marginal at the non-Gaussian fixed point, as in earlier scalar-tensor analyses, so reaching the UV scaling regime requires a tuned infrared choice off 1, and generic traj...

    work page

  2. [2]

    Ten Years of the Fifth Force

    E. Fischbach and C. Talmadge, in31st Rencontres de Moriond: Dark Matter and Cosmology, Quantum Mea- surements and Experimental Gravitation(1996) pp. 443– 451, arXiv:hep-ph/9606249

    work page internal anchor Pith review Pith/arXiv arXiv 1996

  3. [3]

    Fischbach and C

    E. Fischbach and C. L. Talmadge,The Search for Non- Newtonian Gravity(Springer New York, 1998)

    work page 1998

  4. [4]

    Fischbach, D

    E. Fischbach, D. Sudarsky, A. Szafer, C. Talmadge, and S. H. Aronson, Phys. Rev. Lett.56, 3 (1986)

    work page 1986

  5. [5]

    C. M. Will, Living Rev. Rel.17, 4 (2014), arXiv:1403.7377 [gr-qc]

    work page internal anchor Pith review Pith/arXiv arXiv 2014

  6. [6]

    D. J. Kapner, T. S. Cook, E. G. Adelberger,et al., Phys. Rev. Lett.98, 021101 (2007), hep-ph/0611184

    work page internal anchor Pith review Pith/arXiv arXiv 2007

  7. [7]

    E. G. Adelberger, B. R. Heckel, and A. E. Nelson, Prog. Part. Nucl. Phys.62, 102 (2009)

    work page 2009

  8. [8]

    J. D. Andersonet al., Phys. Rev. Lett.62, 1121 (1989)

    work page 1989

  9. [9]

    J. G. Williams, S. G. Turyshev, and D. H. Boggs, Phys. Rev. Lett.93, 261101 (2004), arXiv:gr-qc/0411113

    work page internal anchor Pith review Pith/arXiv arXiv 2004

  10. [10]

    Fienga, J

    A. Fienga, J. Laskar, P. Kuchynka,et al., Celest. Mech. Dyn. Astron.111, 363 (2011)

    work page 2011

  11. [11]

    The String Dilaton and a Least Coupling Principle

    T. Damour and A. M. Polyakov, Nucl. Phys. B423, 532 (1994), hep-th/9401069

    work page internal anchor Pith review Pith/arXiv arXiv 1994

  12. [12]

    Fujii and K.-i

    Y. Fujii and K.-i. Maeda,The Scalar-Tensor Theory of Gravitation(Cambridge University Press, Cambridge, England, 2003)

    work page 2003

  13. [13]

    Selected topics in scalar-tensor theories and beyond

    I. Quiros, Int. J. Mod. Phys. D28, 1930012 (2019), arXiv:1901.08690 [gr-qc]

    work page internal anchor Pith review Pith/arXiv arXiv 2019

  14. [14]

    Zhang, B

    X. Zhang, B. Wang, and R. Niu, Eur. Phys. J. C84, 381 (2024), arXiv:2305.06752 [gr-qc]. 5 FIG. 2. Constraints on Yukawa-type fifth forces in the (α Y , λY ) plane. The orange region is excluded by existing laboratory, geophysical, and Solar System experiments, while the blue region is ruled out by the requirement of non-perturbative UV completeness of sca...

    work page arXiv 2024

  15. [15]

    Huang and X.-M

    L. Huang and X.-M. Deng, Eur. Phys. J. C84, 615 (2024)

    work page 2024

  16. [16]

    Gravity from a Particle Physicists' perspective

    R. Percacci and G. P. Vacca, Class. Quant. Grav.27, 245026 (2010), 0910.5167

    work page internal anchor Pith review Pith/arXiv arXiv 2010

  17. [17]

    Renormalization Group Flow in Scalar-Tensor Theories. I

    G. Narain and R. Percacci, Class. Quant. Grav.27, 075001 (2010), 0911.0386

    work page internal anchor Pith review Pith/arXiv arXiv 2010

  18. [18]

    Asymptotic safety of higher derivative quantum gravity non-minimally coupled with a matter system

    Y. Hamada and M. Yamada, JHEP2017(08), 070, 1703.09033

    work page internal anchor Pith review Pith/arXiv arXiv

  19. [19]

    Search of scaling solutions in scalar-tensor gravity

    R. Percacci and G. P. Vacca, Eur. Phys. J. C75, 188 (2015), 1501.00888

    work page internal anchor Pith review Pith/arXiv arXiv 2015

  20. [20]

    Proper-time functional renormalization in $O(N)$ scalar models coupled to gravity

    A. Bonanno, E. Glaviano, and G. P. Vacca, Proper-time functional renormalization ino(n) scalar models coupled to gravity, arXiv:2508.00807 [hep-th]

    work page internal anchor Pith review Pith/arXiv arXiv

  21. [21]

    The String Landscape, Black Holes and Gravity as the Weakest Force

    N. Arkani-Hamed, L. Motl, A. Nicolis, and C. Vafa, JHEP06, 060, arXiv:hep-th/0601001

    work page internal anchor Pith review Pith/arXiv arXiv

  22. [22]

    The Swampland: Introduction and Review

    E. Palti, Fortsch. Phys.67, 1900037 (2019), arXiv:1903.06239 [hep-th]

    work page internal anchor Pith review Pith/arXiv arXiv 2019

  23. [23]

    Asymptotic Safety of Gravity Coupled to Matter

    R. Percacci and D. Perini, Phys. Rev. D68, 044018 (2003), arXiv:hep-th/0304222

    work page internal anchor Pith review Pith/arXiv arXiv 2003

  24. [24]

    Renormalization Group Flow in Scalar-Tensor Theories. II

    G. Narain and C. Rahmede, Class. Quant. Grav.27, 075002 (2010), arXiv:0911.0394 [hep-th]

    work page internal anchor Pith review Pith/arXiv arXiv 2010

  25. [25]

    B. S. Merzlikin, I. L. Shapiro, A. Wipf, and O. Zanusso, Phys. Rev. D96, 125007 (2017), arXiv:1711.02224 [hep- th]

    work page internal anchor Pith review Pith/arXiv arXiv 2017

  26. [26]

    Asymptotic safety in $O(N)$ scalar models coupled to gravity

    P. Labus, R. Percacci, and G. P. Vacca, Phys. Lett. B 753, 274 (2016), arXiv:1505.05393 [hep-th]

    work page internal anchor Pith review Pith/arXiv arXiv 2016

  27. [27]

    On Exact Proper Time Wilsonian RG Flows

    A. Bonanno, S. Lippoldt, R. Percacci, and G. P. Vacca, Eur. Phys. J. C80, 249 (2020), arXiv:1912.08135 [hep- th]

    work page Pith review arXiv 2020

  28. [28]

    Bonanno and M

    A. Bonanno and M. Reuter, JHEP02, 035, arXiv:hep- th/0410191

    work page arXiv

  29. [29]

    Towards an accurate determination of the critical exponents with the Renormalization Group flow equations

    A. Bonanno and D. Zappala, Phys. Lett. B504, 181 (2001), arXiv:hep-th/0010095

    work page internal anchor Pith review Pith/arXiv arXiv 2001

  30. [30]

    Numerically,k 0 ≃1 eV corresponds to a coarse-graining lengthℓ 0 ∼(ℏc)/k 0 ≈200 nm, well above microscopic interatomic scales, and therefore, appropriate for a con- tinuum, perfect-fluid description of matter

    work page